This paper deals with acceleration processes in the magnetotail and the processes that
enhance particle precipitation from the tail into the ionosphere through electric fields in the …

This paper gives an overview of the insights into the magnetic reconnection process
obtained by in-situ measurements across current sheets found in planetary magnetospheres …

The mechanism that produces energetic electrons during magnetic reconnection is poorly
understood. This is a fundamental process responsible for stellar flares,, substorms,, and …

Magnetic reconnection is an important driver of energetic particles in many astrophysical
phenomena. Using kinetic particle-in-cell simulations, we explore the impact of three …

Particles are accelerated to very high, non-thermal energies during explosive energy-
release phenomena in space, solar, and astrophysical plasma environments. While it has …

Magnetic reconnection in magnetized plasmas represents a change in magnetic field
topology and is associated with a concomitant energization of charged particles that results …

Kinetic simulations of 3D collisionless magnetic reconnection with a guide field show a
dramatic enhancement of energetic electron production when compared with 2D systems. In …

We report evidence for reconnection between colliding reconnection jets in a compressed
current sheet at the center of a magnetic flux rope at Earth's magnetopause. The …

Observations of Particle Acceleration in Magnetic Reconnection–driven Turbulence -
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Particles are accelerated to very high, non-thermal energies in solar and space plasma
environments. While energy spectra of accelerated electrons often exhibit a power law, it …